A) Iron. B) Oxygen. C) Hydrogen. D) Helium.
A) Interactions between charged particles. B) Radioactive decay. C) Geometric shapes of galaxies. D) Lack of energy.
A) Increase the speed of light. B) Can create new colors. C) Can cause light to become polarized. D) Can absorb all light.
A) An area of low pressure. B) A flat line in a spectrograph. C) A sudden increase in pressure and temperature. D) A change in the structure of magnetic fields.
A) Causes instability in stars. B) Enhances the transport of energy and particles. C) Reduces the speed of light. D) Produces new elements.
A) The speed of light. B) Propagation of Alfvén waves. C) The size of a galaxy. D) The movement of planets.
A) Jupiter B) Andromeda Galaxy C) Saturn D) The Sun
A) A hot area in the center of the Sun. B) A natural light display caused by the interaction of charged particles with a planet's magnetic field. C) A type of asteroid. D) A formation of ice on comets.
A) Through observations, simulations, and laboratory experiments. B) By sending rockets into space. C) Through mental visualization. D) Through direct physical contact.
A) They emit strong magnetic fields. B) They shield galaxies from cosmic rays. C) They are the largest structures in the universe and act as highways for gas and galaxies. D) They have no significant role in space.
A) Opposing magnetic field lines breaking and reconnecting. B) Collision of planets. C) Sudden bursts of radiation. D) Expansion of the universe.
A) Boomerang Nebula B) Earth's poles C) The center of a star D) The Sun's surface
A) A change in the speed of light. B) A massive release of plasma and magnetic fields from a star's corona. C) A sudden brightening of a distant galaxy. D) A warp in the space-time continuum.
A) By repelling each other due to electric charge. B) By blocking cosmic rays. C) By emitting strong radio waves. D) By collapsing under gravity and undergoing nuclear fusion.
A) Mars B) Saturn C) Jupiter D) Earth
A) By detecting gravitational waves from black holes. B) By studying the behavior of accretion disks around black holes. C) By measuring the temperature on black hole surfaces. D) By observing the shape of black holes. |